DocumentCode
3365674
Title
Convolution calculation of differential cross sections of ring effect
Author
Han, Dong ; Chen, Liangfu ; Wu, Weimin ; Li, Shenshen ; Yu, Chao
Author_Institution
State Key Lab. of Remote Sensing Sci., Beijing Normal Univ., Beijing, China
fYear
2010
fDate
25-30 July 2010
Firstpage
1137
Lastpage
1140
Abstract
The Ring effect refers to the filling in of Fraunhofer lines, which is known as solar absorption lines, caused almost entirely by Rotational Raman scattering. The Rotational Raman scattering by N2 and O2 in the atmosphere is the main factor that leads to Ring effect. Basically, the Ring effect is considered as a pseudo-absorption process in retrieval of trace gas constituents in atmosphere. The solar spectrum measured by OMI/AURA is convolved with rotational Raman cross sections of N2 and O2, divided by the original solar spectrum, with a cubic polynomial subtracted off, to create a differential Ring spectrum. This method has been suggested in order to obtain an effective differential Ring cross-section for the DOAS fitting process. The differential Ring spectrum could be used to improve the accuracy of the retrieval of the trace gases concentration. The results have been in basic agreement with the corresponding results calculated with RTM, and the R2 statistic is 0.9663.Next, the differential Ring spectrum calculated with rotational Raman cross sections of atmosphere in the fixed wavelength of 410nm and 488nm are derived. The results with the fixed wavelength have been also in basic agreement with the corresponding results calculated with RTM, and the R2 statistics are 0.9624 and 0.9639 respectively. At last but not the least, the computational complexity calculated at fixed wavelength of 410nm or of 488nm is 0.128% of that calculated with wavelengths from 410nm to 488nm.
Keywords
Raman spectra; convolution; solar spectra; DOAS fitting process; Fraunhofer line; Raman cross section; convolution calculation; cubic polynomial; differential cross section; differential ring spectrum; pseudo-absorption process; rotational Raman scattering; solar absorption line; wavelength 410 nm; wavelength 488 nm; Absorption; Atmosphere; Atmospheric measurements; Convolution; Instruments; Pollution measurement; Raman scattering; DOAS; N2 and O2 ; Ring effect; rotational Raman scattering; trace gas;
fLanguage
English
Publisher
ieee
Conference_Titel
Geoscience and Remote Sensing Symposium (IGARSS), 2010 IEEE International
Conference_Location
Honolulu, HI
ISSN
2153-6996
Print_ISBN
978-1-4244-9565-8
Electronic_ISBN
2153-6996
Type
conf
DOI
10.1109/IGARSS.2010.5653498
Filename
5653498
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